Search Publications

Planck 2018 results. VI. Cosmological parameters
DOI: 10.1051/0004-6361/201833910 Bibcode: 2020A&A...641A...6P

Kim, J.; Miville-Deschênes, M. -A.; Boulanger, F. +179 more

We present cosmological parameter results from the final full-mission Planck measurements of the cosmic microwave background (CMB) anisotropies, combining information from the temperature and polarization maps and the lensing reconstruction. Compared to the 2015 results, improved measurements of large-scale polarization allow the reionization opti…

2020 Astronomy and Astrophysics
eHST 15139
DYNESTY: a dynamic nested sampling package for estimating Bayesian posteriors and evidences
DOI: 10.1093/mnras/staa278 Bibcode: 2020MNRAS.493.3132S

Speagle, Joshua S.

We present DYNESTY, a public, open-source, PYTHON package to estimate Bayesian posteriors and evidences (marginal likelihoods) using the dynamic nested sampling methods developed by Higson et al. By adaptively allocating samples based on posterior structure, dynamic nested sampling has the benefits of Markov chain Monte Carlo (MCMC) algorithms tha…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 1620
Planck 2018 results. I. Overview and the cosmological legacy of Planck
DOI: 10.1051/0004-6361/201833880 Bibcode: 2020A&A...641A...1P

Kim, J.; Miville-Deschênes, M. -A.; Boulanger, F. +192 more

The European Space Agency's Planck satellite, which was dedicated to studying the early Universe and its subsequent evolution, was launched on 14 May 2009. It scanned the microwave and submillimetre sky continuously between 12 August 2009 and 23 October 2013, producing deep, high-resolution, all-sky maps in nine frequency bands from 30 to 857 GHz.…

2020 Astronomy and Astrophysics
XMM-Newton 1575
H0LiCOW - XIII. A 2.4 per cent measurement of H0 from lensed quasars: 5.3σ tension between early- and late-Universe probes
DOI: 10.1093/mnras/stz3094 Bibcode: 2020MNRAS.498.1420W

Treu, Tommaso; Marshall, Philip J.; Sonnenfeld, Alessandro +23 more

We present a measurement of the Hubble constant (H0) and other cosmological parameters from a joint analysis of six gravitationally lensed quasars with measured time delays. All lenses except the first are analysed blindly with respect to the cosmological parameters. In a flat Λ cold dark matter (ΛCDM) cosmology, we find $H_{0} = 73.3_{…

2020 Monthly Notices of the Royal Astronomical Society
eHST 1089
The Pan-STARRS1 Database and Data Products
DOI: 10.3847/1538-4365/abb82d Bibcode: 2020ApJS..251....7F

Price, P. A.; Rest, A.; Saglia, R. P. +36 more

This paper describes the organization of the database and the catalog data products from the Pan-STARRS1 3π Steradian Survey. The catalog data products are available in the form of an SQL-based relational database from MAST, the Mikulski Archive for Space Telescopes at STScI. The database is described in detail, including the construction of the d…

2020 The Astrophysical Journal Supplement Series
Gaia 784
The Solar Orbiter mission. Science overview
DOI: 10.1051/0004-6361/202038467 Bibcode: 2020A&A...642A...1M

Williams, D.; Livi, S.; Peter, H. +32 more


Aims: Solar Orbiter, the first mission of ESA's Cosmic Vision 2015-2025 programme and a mission of international collaboration between ESA and NASA, will explore the Sun and heliosphere from close up and out of the ecliptic plane. It was launched on 10 February 2020 04:03 UTC from Cape Canaveral and aims to address key questions of solar and …

2020 Astronomy and Astrophysics
SolarOrbiter Ulysses 754
New physics in light of the H0 tension: An alternative view
DOI: 10.1103/PhysRevD.102.023518 Bibcode: 2020PhRvD.102b3518V

Vagnozzi, Sunny

The strong discrepancy between local and early-time (inverse distance ladder) estimates of the Hubble constant H0 could be pointing towards new physics beyond the concordance Λ CDM model. Several attempts to address this tension through new physics rely on extended cosmological models, featuring extra free parameters beyond the six Λ CD…

2020 Physical Review D
eHST 431
Painting a portrait of the Galactic disc with its stellar clusters
DOI: 10.1051/0004-6361/202038192 Bibcode: 2020A&A...640A...1C

Castro-Ginard, A.; Jordi, C.; Casamiquela, L. +10 more

Context. The large astrometric and photometric survey performed by the Gaia mission allows for a panoptic view of the Galactic disc and its stellar cluster population. Hundreds of stellar clusters were only discovered after the latest Gaia data release (DR2) and have yet to be characterised.
Aims: Here we make use of the deep and homogeneous …

2020 Astronomy and Astrophysics
Gaia 410
The Sloan Digital Sky Survey Quasar Catalog: Sixteenth Data Release
DOI: 10.3847/1538-4365/aba623 Bibcode: 2020ApJS..250....8L

Brandt, W. N.; Pâris, Isabelle; Petitjean, Patrick +34 more

We present the final Sloan Digital Sky Survey IV (SDSS-IV) quasar catalog from Data Release 16 of the extended Baryon Oscillation Spectroscopic Survey (eBOSS). This catalog comprises the largest selection of spectroscopically confirmed quasars to date. The full catalog includes two subcatalogs (the current versions are DR16Q_v4 and DR16Q_Superset_…

2020 The Astrophysical Journal Supplement Series
Gaia XMM-Newton 408
APOGEE Data and Spectral Analysis from SDSS Data Release 16: Seven Years of Observations Including First Results from APOGEE-South
DOI: 10.3847/1538-3881/aba592 Bibcode: 2020AJ....160..120J

Bizyaev, Dmitry; Bovy, Jo; Cunha, Katia +20 more

The spectral analysis and data products in Data Release 16 (DR16; 2019 December) from the high-resolution near-infrared Apache Point Observatory Galactic Evolution Experiment (APOGEE)-2/Sloan Digital Sky Survey (SDSS)-IV survey are described. Compared to the previous APOGEE data release (DR14; 2017 July), APOGEE DR16 includes about 200,000 new ste…

2020 The Astronomical Journal
Gaia 404